Spin Down of Rotating Compact Magnetized Strange Stars in General Relativity

Spin Down of Rotating Compact Magnetized Strange Stars in General Relativity

We find that in general relativity slow down of the pulsar rotation due to the magnetodipolar radiation is more faster for the strange star with comparison to that for the neutron star of the same mass. Comparison with astrophysical observations on pulsars spindown data may provide an evidence for t...

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Veröffentlicht in:arXiv.org 2011-10
Hauptverfasser: Ahmedov, B J, Ahmedov, B B, Abdujabbarov, A A
Format: Artikel
Sprache:eng
Schlagworte:
Neutron stars
Neutrons
Physics - Solar and Stellar Astrophysics
Pulsars
Relativity
Theory of relativity
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Zusammenfassung:We find that in general relativity slow down of the pulsar rotation due to the magnetodipolar radiation is more faster for the strange star with comparison to that for the neutron star of the same mass. Comparison with astrophysical observations on pulsars spindown data may provide an evidence for the strange star existence and, thus, serve as a test for distinguishing it from the neutron star.
ISSN:2331-8422
DOI:10.48550/arxiv.1110.6586